9056: showed a long, thin tail that
was visible in C3 images (which showed a small head that
peaked at mag about 2-3
and a tail length of about 1 degree) as well as in C2
SOHO images and in SECCHI COR2-A and COR2-B images

8883: peaked at mag about 3 with a dense, wide tail
about 45" long on June 8.171 UT; while the comet's
"head" disappeared
at about June 8.181, the tail was still visible at June
8.917 (when it had extended into a diffuse arc of
apparent length around
1.5 deg), and this comet was also visible in coronagraphs
on both STEREO spacecraft

8982: was one of the brightest comets
seen by SOHO (saturating slightly in both LASCO cameras,
with estimated peak
magnitude about 1-2), appearing as a bright teardrop in
C3 images and having a partly-forked, "thick"
tail about 0.5 long
in C2 images; both SECCHI COR cameras also imaged C/2008
K4, with the tail appearing somewhat thinner in the
COR2A images and showing the slight "fork" in
the COR2B images

8984: was teardrop-shaped (mag about
3-4) in C3 images, and showed a diffuse tail about 0.25
deg long in C2 images
(the tail also similarly visible in SECCHI COR2-A images,
and as somewhat fainter and shorter in COR2-B images)

8985: was very bright (mag about 4.5)
and elongated in C3 images, and showed a diffuse tail
about 0.5 deg long in C2 images
(where it appeared headless inside about 6 solar radii
(apparent); SECCHI COR2-A images on July 3-4 showed a
thin tail
much like that seen in C2 images, and a tail also was
seen to form in the last images obtained with the COR2-B
camera on July 4.

9006: an additional near-sun
Kracht-group presumed comet was found by R. Kracht on
SOHO website images.
C/2008 R7 was stellar in appearance in C3, C2, and COR2-A
images, peaking at mag about 5.5 around Sept. 6.83 UT.

9056: showed a long, thin tail that
was visible in C3 images (which showed a small head that
peaked at mag about 2-3 and
a tail length of about 1 degree) as well as in C2 SOHO
images and in SECCHI COR2-A and COR2-B images

9070:was bright
(mag about 4) with a short tail in LASCO C3 images, while
it showed a short tail and faded quickly in C2 images;
this comet was also detected in STEREO COR2-A and COR2-B
images with a tail about 0.3 deg long

9065: was stellar in appearance (mag
about 6.5) in C3 images but quite large and very
condensed with no visible tail in C2 images;
COR2-A STEREO images show a bright starlike head and a
very faint, thin tail.

9057: may have been around mag 6 or
6.5, appeared as a somewhat-long thin streak with no
discernable head or coma in COR2-A
images;in COR2-B images, the comet appeared much more
condensed (possibly slightly diffuse and with a hint of a
barely detectable tail)

8883: peaked at mag about 3 with a dense, wide tail
about 45" long on June 8.171 UT; while the comet's
"head" disappeared
at about June 8.181, the tail was still visible at June
8.917 (when it had extended into a diffuse arc of
apparent length around
1.5 deg), and this comet was also visible in coronagraphs
on both STEREO spacecraft

8982: was one of the brightest comets
seen by SOHO (saturating slightly in both LASCO cameras,
with estimated peak
magnitude about 1-2), appearing as a bright teardrop in
C3 images and having a partly-forked, "thick"
tail about 0.5 long
in C2 images; both SECCHI COR cameras also imaged C/2008
K4, with the tail appearing somewhat thinner in the
COR2A images and showing the slight "fork" in
the COR2B images

8984: was teardrop-shaped (mag about
3-4) in C3 images, and showed a diffuse tail about 0.25
deg long in C2 images
(the tail also similarly visible in SECCHI COR2-A images,
and as somewhat fainter and shorter in COR2-B images)

8985: was very bright (mag about 4.5)
and elongated in C3 images, and showed a diffuse tail
about 0.5 deg long in C2 images
(where it appeared headless inside about 6 solar radii
(apparent); SECCHI COR2-A images on July 3-4 showed a
thin tail
much like that seen in C2 images, and a tail also was
seen to form in the last images obtained with the COR2-B
camera on July 4.

9056: showed a long, thin tail that
was visible in C3 images (which showed a small head that
peaked at mag about 2-3 and
a tail length of about 1 degree) as well as in C2 SOHO
images and in SECCHI COR2-A and COR2-B images

9070:was bright
(mag about 4) with a short tail in LASCO C3 images, while
it showed a short tail and faded quickly in C2 images;
this comet was also detected in STEREO COR2-A and COR2-B
images with a tail about 0.3 deg long

9057: may have been around mag 6 or
6.5, appeared as a somewhat-long thin streak with no
discernable head or coma in COR2-A images;
in COR2-B images, the comet appeared much more condensed
(possibly slightly diffuse and with a hint of a barely
detectable tail)

9056: showed a long, thin tail that
was visible in C3 images (which showed a small head that
peaked at mag about 2-3 and a tail length of about 1
degree) as well as in C2 SOHO images
and in SECCHI COR2-A and COR2-B images

9070:was bright
(mag about 4) with a short tail in LASCO C3 images, while
it showed
a short tail and faded quickly in C2 images; this comet
was also detected in STEREO COR2-A
and COR2-B images with a tail about 0.3 deg long